50 research outputs found

    Rapid changes in ice core gas records Part 2: Understanding the rapid rise in atmospheric CO2 at the onset of the BĂžlling/AllerĂžd

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    During the last glacial/interglacial transition the Earth's climate underwent rapid changes around 14.6 kyr ago. Temperature proxies from ice cores revealed the onset of the Bþlling/Allerþd (B/A) warm period in the north and the start of the Antarctic Cold Reversal in the south. Furthermore, the B/A is accompanied by a rapid sea level rise of about 20 m during meltwater pulse (MWP) 1A, whose exact timing is matter of current debate. In situ measured CO<sub>2</sub> in the EPICA Dome C (EDC) ice core also revealed a remarkable jump of 10&plusmn;1 ppmv in 230 yr at the same time. Allowing for the age distribution of CO<sub>2</sub> in firn we here show, that atmospheric CO<sub>2</sub> rose by 20–35 ppmv in less than 200 yr, which is a factor of 2–3.5 larger than the CO<sub>2</sub> signal recorded in situ in EDC. Based on the estimated airborne fraction of 0.17 of CO<sub>2</sub> we infer that 125 Pg of carbon need to be released to the atmosphere to produce such a peak. Most of the carbon might have been activated as consequence of continental shelf flooding during MWP-1A. This impact of rapid sea level rise on atmospheric CO<sub>2</sub> distinguishes the B/A from other Dansgaard/Oeschger events of the last 60 kyr, potentially defining the point of no return during the last deglaciation

    Heterogeneous deformation during electromagnetic ring expansion test

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    High speed forming methods become attractive in manufacturing and it significantl reduces the cost and energy requirements. Conventional manufacturing processes such as forging, forming, stamping and cutting of metals typically involve a strain rate of 10 2 – 10 4 s-1 which includes high energy rate fabrication (HERF) methods [1]. During advanced manufacturing methods such as high speed forming and high speed welding processes, certain local regions (e.g. interfaces) of materials could also experience significantly high strain rate (> 10 4 s-1). In order to understand the physical behaviours of materials and to design/control/optimise, such manufacturing processes that require an appropriate technique to capture the material’s viscoplastic property under the high strain rate deformation. Therein, the electromagnetic ring expansion test becomes a promising method to characterize the material behaviours under the high strain rate deformation. The ring expansion is caused by Lorentz force that is generated due to the magnetic induction on the ring. However, the realistic nature of the electromagnetic ring expansion test is quite complex because of the coupling physics between electromagnetic-thermal-mechanical components. Therefore, in this study we evaluate certain controlling parameters which govern the fundamental behaviour of the electromagnetic ring expansion test. Particularly the rotation and inhomogeneous deformation of the ring are noticeably observed and these phenomena require extra attention

    TALDICE-1 age scale of the Talos Dome deep ice core, East Antarctica

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    A new deep ice core drilling program, TALDICE, has been successfully handled by a European team at Talos Dome, in the Ross Sea sector of East Antarctica, down to 1620m depth. Using stratigraphic markers and a new inverse method, we produce the first official chronology of the ice core, called TALDICE-1. We show that it notably improves an a priori chronology resulting from a one-dimensional ice flow model. It is in agreement with a posteriori controls of the resulting accumulation rate and thinning function along the core. An absolute uncertainty of only 300 yr is obtained over the course of the last deglaciation. This uncertainty remains lower than 600 yr over Marine Isotope Stage 3, back to 50 kyr BP. The phasing of the TALDICE ice core climate record with respect to the central East Antarctic plateau and Greenland records can thus be determined with a precision allowing for a discussion of the mechanisms at work at submillennial time scales

    Abrupt Ice Age Shifts in Southern Westerlies and Antarctic Climate Forced from the North

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    The Southern Hemisphere (SH) mid-latitude westerly winds play a central role in the global climate system via Southern Ocean upwelling, carbon exchange with the deep ocean, Agulhas Leakage, and Antarctic ice sheet stability. Meridional shifts in the SH westerlies have been hypothesized in response to abrupt North Atlantic Dansgaard-Oeschger (DO) climatic events of the last ice age, in parallel with the well-documented shifts of the intertropical convergence zone. Shifting moisture pathways to West Antarctica are consistent with this view, but may represent a Pacific teleconnection pattern. The full SH atmospheric-circulation response to the DO cycle, as well as its impact on Antarctic temperature, have so far remained unclear. Here we use five volcanically-synchronized ice cores to show that the Antarctic temperature response to the DO cycle can be understood as the superposition of two modes: a spatially homogeneous oceanic “bipolar seesaw” mode that lags Northern Hemisphere (NH) climate by about 200 years, and a spatially heterogeneous atmospheric mode that is synchronous with NH abrupt events. Temperature anomalies of the atmospheric mode are similar to those associated with present-day Southern Annular Mode (SAM) variability, rather than the Pacific South America (PSA) pattern. Moreover, deuterium excess records suggest a zonally coherent migration of the SH westerlies over all ocean basins in phase with NH climate. Our work provides a simple conceptual framework for understanding the circum-Antarctic temperature response to abrupt NH climate change. We provide observational evidence for abrupt shifts in the SH westerlies, with ramifications for global ocean circulation and atmospheric CO₂. These coupled changes highlight the necessity of a global, rather than a purely North Atlantic, perspective on the DO cycle

    Speciation analysis of iodine and bromine at picogram-per-gram levels in polar ice

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    Iodine and bromine species participate in key atmospheric reactions including the formation of cloud con- densation nuclei and ozone depletion. We present a novel method coupling a high-performance liquid chromatogra- phy with ion chromatography and inductively coupled plas- ma mass spectrometry, which allows the determination of iodine (I) and bromine (Br) species (IO3−, I−, Br−, BrO3−) at the picogram-per-gram levels presents in Antarctic ice. Chromatographic separation was achieved using an ION- PAC¼ AS16 Analytical Column with NaOH as eluent. Detection limits for I and Br species were 5 to 9 pg g−1 with an uncertainty of less than 2.5% for all considered species. Inorganic iodine and bromine species have been determined in Antarctic ice core samples, with concentrations close to the detection limits for iodine species, and approximately 150 pg g−1 for Br−. Although iodate (IO3−) is the most abundant iodine species in the atmosphere, only the much rarer iodide (I−) species was present in Antarctic Holocene ice. Bromine was found to be present in Antarctic ice as Br−

    Abrupt rise in atmospheric CO2 at the onset of the BĂžlling/AllerĂžd: in-situ ice core data versus true atmospheric signal

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    During the last glacial/interglacial transition the Earth's climate underwent abrupt changes around 14.6 kyr ago. Temperature proxies from ice cores revealed the onset of the BĂžlling/AllerĂžd (B/A) warm period in the north and the start of the Antarctic Cold Reversal in the south. Furthermore, the B/A was accompanied by a rapid sea level rise of about 20 m during meltwater pulse (MWP) 1A, whose exact timing is a matter of current debate. In-situ measured CO2 in the EPICA Dome C (EDC) ice core also revealed a remarkable jump of 10±1 ppmv in 230 yr at the same time. Allowing for the modelled age distribution of CO2 in firn, we show that atmospheric CO2 could have jumped by 20–35 ppmv in less than 200 yr, which is a factor of 2–3.5 greater than the CO2 signal recorded in-situ in EDC. This rate of change in atmospheric CO2 corresponds to 29–50% of the anthropogenic signal during the last 50 yr and is connected with a radiative forcing of 0.59–0.75 W m−2. Using a model-based airborne fraction of 0.17 of atmospheric CO2, we infer that 125 Pg of carbon need to be released into the atmosphere to produce such a peak. Available ÎŽ13CO2 data are neutral, whether the source of the carbon is of marine or terrestrial origin. We hypothesise that most of the carbon might have been activated as a consequence of continental shelf flooding during MWP-1A. We furthermore plan to challange our hypothesis by comparing its typical 14C signature with so far unpublished high resolution 14C data from Tahiti corals (Durant et al., 2010, Geophysical Research Abstracts, 12, EGU2010-12689-1).This potential impact of rapid sea level rise on atmospheric CO2 might define the point of no return during the last deglaciation

    Study of self-shielding in dpa calculations

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    International audienceSelf-shielding due to the resonance of cross sections influences the neutron spectrum. Mature treatment of the self-shielding has been developed in deterministic neutron transport codes. However, the correction of both neutron flux and cross sections cannot ensure the accuracy of calculated Displacement per Atom (DPA), which depends not only on cross sections, but also the corresponding recoil energies of the Primary Knocked-on Atom (PKA). The present study focuses on 56Fe because it is the most abundant isotope in the stainless steel, which is the material for the reactor pressure vessel in light water reactors and that of the fuel cladding in fast reactors. Due to the temperature dependence of cross sections, the temperature effect is firstly analyzed. Results show that the Doppler effect has small influence on DPA calculation for 56Fe. 33-group and 1968-group DPA cross sections are then used to investigate the influence of the self-shielding on the DPA calculation. The effect of the self-shielding on DPA rate calculation is examined in the fuel cladding in the ASTRID inner core. The contribution of the elastic scattering, inelastic scattering, and disappearance reactions to total DPA are 82.7percent, 17.1percent, and 0.1percent, respectively. Relative and respective reductions are 11.3percent, 5.9percent, and 20.5percent by taking the self-shielding into account. The calculation of DPA is not summable after self-shielding correction because the DPA calculated by total cross sections is 2.3percent lower the sum of the above three components
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